\begin{table}%t2
\caption{\label{tab2}List of possible additional faint counterparts to CMaX sources.}
\par
%\centerline
{\small
\begin{tabular}{lcccccccccccc}
\hline\hline
\noalign{\smallskip}
CMaX & RA & Dec & $R_{\rm int}$ & $R$ & $V-R$ & $R-I$ & $J_{\rm int}$ & $J$ & $J-H^d$ & $H-K^d$ & Age & Mass \\
& J2000& J2000& (mag) & (mag) & (mag) &(mag)& (mag) & (mag) &(mag) & (mag)& (Myr) & ($M_{\odot}$) \\
%\noalign{\smallskip}
\hline
\noalign{\smallskip}
15-1 & 7 00 13.364 & $-11$ 18 53.43 & 16.5$^e$& 17.1$^a$ & 0.29 & 1.08$^b$ &14.4$^e$ &14.77 & 0.70 $\pm$ 0.06 & 0.19 $\pm$ 0.07 & 10--20 & 0.5--1.0 \\
15-2 & 7 00 13.509 & $-11$ 19 11.14 & &18.3 & 0.70 & 0.78 & &16.84 & 0.66 $\pm$ 0.28 & 0.81 $\pm$ 0.28$^c$ & ?? & ?? \\
15-3 & 7 00 15.325 & $-11$ 18 58.56 & &18.6 & 0.73 & 0.79 & &16.71 & 0.38 $\pm$ 0.29 & 0.68 $\pm$ 0.34$^c$ & ?? & ?? \\
15-4 & 7 00 15.378 & $-11$ 19 3.78 & &19.7 & 1.6 & 1.56$^b$ & &16.45 & 0.76 $\pm$ 0.19 & 0.29 $\pm$ 0.24 &10--20 & 0.1--0.5 \\
\hline 
\noalign{\smallskip} 
17N & 7 00 18.724 & $-11$ 22 24.02 & & 18.8 & 0.89 & 0.90$^b$ & &16.59 & 0.50$\pm$ 0.25 & 0.58$\pm$ 0.30$^c$  & ?? & ?? \\
17S1 & 7 00 18.806 & $-11$ 23 16.10 & 16.9$^e$&17.1 & 0.9 & 0.79$^b$ &15.4$^e$ &15.58 & 0.77 $\pm$ 0.1 & 0.14 $\pm$ 0.14 & 20--50 & 0.5--1.0 \\
17S2 & 7 00 18.886 & $-11$ 23 23.67 & &19.2 & 1.22 & 1.15$^b$ & &16.71 & 0.89 $\pm$ 0.22 & 0.14 $\pm$ 0.29 & 20--50 & 0.1--0.5 \\
\hline
\noalign{\smallskip}
37-1 & 7 01 22.297 & $-11$ 09 9.29 & &17.7 & 0.9 & 0.97$^b$ & &16.18 & 0.65 $\pm$ 0.15 & -0.1 $\pm$ 0.24 & 10--20 & 0.5--1.0 \\
37-2 & 7 01 23.560 & $-11$ 08 26.77 & &18.2 & 1.61 & 1.67$^b$ & &15.71 & 0.73 $\pm$ 0.12 & 0.07 $\pm$ 0.16 & 1--2 & 0.5--1.0 \\
37-3 & 7 01 24.356 & $-11$ 09 03.00 & 15.9$^e$&16.3$^a$ & -0.3 & 0.88$^b$ &14.3$^e$ &14.78 & 0.55 $\pm$ 0.06 & 0.11 $\pm$ 0.08 & 5--10 & 0.5--1.0 \\
\hline 
\noalign{\smallskip} 
42-1 & 7 01 35.313 & $-11$ 10 12.23 & &17.2 & 0.73 & 0.73$^b$ & && & & 20--50 & 0.5--1.0 \\
42-2 & 7 01 35.437 & $-11$ 10 44.07 & 15.6$^e$&15.7$^a$ & -0.08 & 0.86$^b$ & 13.9$^e$ & 14.44 & 0.35 $\pm$ 0.06 & 0.08 $\pm$ 0.08 & 2--5 & 0.5--1.0 \\
42-3 & 7 01 35.473 & $-11$ 10 14.46 & &16.4 & 0.74 & 0.71$^b$ & &14.70 & 0.73 $\pm$ 0.08 & 0.21 $\pm$ 0.08 & 10--20 & 0.5--1.0 \\
\hline
\noalign{\smallskip} 
55N & 7 02 8.021 & $-11$ 16 17.65 & 18.2$^e$&18.2$^a$ & 0.98 & 1.08$^b$ &15.6$^e$ &15.67 & 0.64 $\pm$ 0.1 & 0.35 $\pm$ 0.13 & 10--20 & 0.1--0.5 \\
55S & 7 02 8.139 & $-11$ 17 35.46 & &18.9  & 0.6 & 0.74 & &16.46 & 0.73 $\pm$ 0.2 & 0.58 $\pm$ 0.22$^c$ & ?? & ?? \\
\hline
\end{tabular}}
\medskip
Notes: (a) Magnitudes adopted from the NOMAD and/or USNO catalogues, when the estimation from
\textit{Gemini} images are unavailable, due to saturation; (b) counterparts selected according to the $R-I$ excess; (c) counterparts having $H-K$ excess; (d) the 2MASS catalogue was used to obtain the $JHK$ magnitudes, for which error bars are provided; (e) $R_{\rm int}$ and $J_{\rm int}$ represent the ``integrated'' magnitudes (see Sect.~4.2), which are shown together with the brightest object of each group. 
\end{table}